{"paper":{"title":"The radio-loud AGN population at z>~1 in the COSMOS field. I. Selection and Spectral Energy Distributions","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2, (2) Technion, 3), (4) INAF-Osservatorio Astronomico di Torino, (5) Space Telescope Science Institute, 6, (6) INAF-Istituto di Radio Astronomia, 7), (7) Johns Hopkins University, 8, (8) INAF-Osservatorio Astronomico di Brera, 9) ((1) SISSA, (9) INFN-Sezione di Trieste), Alessandro Capetti (4), Annalisa Celotti (1, Baltimore, Bologna, Haifa (3) University of Haifa, Marco Chiaberge (5, Ranieri D. Baldi (1, Trieste","submitted_at":"2014-05-07T19:23:15Z","abstract_excerpt":"We select a sample of radio galaxies at high redshifts (z>~1) in the COSMOS field, by cross-matching optical/infrared images with the FIRST radio data. The aim of this study is to explore the high-z radio-loud (RL) AGN population at much lower luminosities than the classical samples of distant radio sources and similar to those of the local population of radio galaxies. The wide multiwavelength coverage provided by the COSMOS survey allows us to derive their Spectral Energy Distributions (SEDs). The SED modeling with stellar and dust components (with our code 2SPD) returns several important qu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.1711","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}